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The Laser W akefield Accelerator (LW FA): towards a compact light source Mark Wiggins Contents ALPHA-X project W hat is a L W FA? Motivation: quality electron beams and light sources The ALPHA-X beam line: experimental


  1. The Laser W akefield Accelerator (LW FA): towards a compact light source Mark Wiggins

  2. Contents • ALPHA-X project • W hat is a L W FA? • Motivation: quality electron beams and light sources • The ALPHA-X beam line: experimental setup • Experimental results: pointing and energy stability, charge, energy spread, emittance, bunch length • L W FA and beam transport simulations • O utlook for free-electron laser (FEL) driven by L W FA beam • Summary

  3. ALPHA- X Project Advanced Laser Plasma High-energyAccelerators towards X-rays • BasicTechnology grant (2002) and EPSRC grant (2007) • Consortium of U.K. research teams (Stage 2) U. U. U. U. Cockcroft Strathclyde St. Andrews Dundee Institute Abertay D. Jaroszynski A. Cairns A. Gillespie M. Poole Dundee B. Bingham R. Tucker A. MacLeod K. Ledingham P. McKenna Partners – L. Silva & T. Mendonca (IST), B. Cros (UPS - LPGP), W. Leemans (LBNL), B. van der Geer & M. de Loos (Pulsar Phys), G. Shvets (UTA), J. Zhang (CAS) And numerous collaborators

  4. ALPHA- X Project Group Leader: Prof. Dino Jaroszynski Experiments: Riju Issac, Gregor Welsh, Enrico Brunetti, Gregory Vieux PhDs: Richard Shanks, Maria Pia Anania, Silvia Cipiccia, Salima Abuazoum, Grace Manahan, Constantin Aniculaesei, Anna Subiel, David Grant Theory: Bernhard Ersfeld, Ranaul Islam, Gaurav Raj, Adam Noble PhDs: John Farmer, Sijia Chen, Ronan Burgess, Yevgen Kravets Technicians: David Clark, Tom McCanny Visiting Professor: Rodolfo Bonifacio Scottish Universities Physics Alliance

  5. The LWFA • Tajima & Dawson PRL 43 , 267 (1979). ion bubble laser • Intense femtosecond laser propagating in underdense plasma. • Relativistically self-guided channel. • Ponderomotive force leads to charge separation and plasma density wake. • Electrons trapped at back of bubble self-injected electron bunch and accelerated in the very large undergoing betatron oscillations electrostatic fields. • Electron velocity (~ c ) > laser group velocity and electrons catch up on laser. • Energy at dephasing length:

  6. Motivation User Facilities: SSRL synchrotron LCLS X-ray FEL RF Linac: 3.2 km long 50 GeV electrons 16 MeV/m gradient ALPHA-X • Conventional synchrotrons and FELs are very large Length ~10 m • A L W FA-driven light source is ultra-compact • Accelerating gradient ~100 GeV/m • Great uses: short pulses, small source sizes • W ider accessibility

  7. Conventional v Plasma Accelerators RF Cavities Plasma waves • Max. E field ~100 MV/m • 1000 times smaller & cheaper • Limited by breakdown • 1 GeV in 33 mm capillary (LBN L 2006) Strathclyde Capillary

  8. Our goal L W FAs to date • High charge density: 10’s of pC in inferred ~ 10 fs (peak current I ~ kA) inferred ε N ~ few π mm mrad (no direct measurements) • Low emittance: • Significant relative energy spread σ γ / γ ~ 1 – 2% at best • X-ray FEL needs σ γ / γ ~0.1% • We are looking to produce high quality electron beams (high I , low ε N , low σ γ / γ ) • And to apply them in useful ways: • Medical imaging • Ultrafast probing • Detector development for nuclear physics • Strathclyde/Glasgow/Institute for Cancer Research project (e − beam therapy) • Future plans at the end...

  9. Synchrotron / undulator radiation • Relativistic electrons in a magnetic field follow a curved trajectory and i.e. they are accelerated. • Radiation emitted into a narrow cone (lab frame of reference). • Single magnet: synchrotron, Magnet array: undulator or wiggler. N periods Undulator Δ λ 1 1 = θ ≅ λ cen γ N N period λ u • Undulator Equation λ ⎛ ⎞ 2 K ⎜ ⎟ λ = + + θ γ 2 2 1 u ⎜ ⎟ where h is the harmonic order and K = λ u eB/2 π m 0 c < 1 γ 2 2 2 ⎝ ⎠ h

  10. LWFA undulator radiation • J ena / Strathclyde / Stellenbosch experiment Schlenvoigt et al., N ature Phys. 4 , 130 (2008) • 55-70 MeV electrons • VIS/IR synchrotron radiation Gallacher et al., Phys. Plasmas 16 , 093102 (2009)

  11. LWFA undulator radiation • MPQ / FZD / O xford experiment • 150-210 MeV electrons • XUV synchrotron radiation Fuchs et al., N ature Phys. 5, 826 (2009) Free-electron laser for 10 6 – 10 8 increase in photon output • N ext step: ε n < λγ /4 π and σ γ / γ < ρ • High FEL gain criteria: • N eed the beam quality and good transport...

  12. ALPHA- X Beam Line Accelerator PMQs Pepper pot Pellicle Electron EMQs Spectrometer Undulator λ 0 = 800 nm, E = 900 mJ , τ = 35 fs, P = 26 TW, I = 2 × 10 18 W cm -2 , initial a 0 = 1.0 • Laser: helium, 2 mm nozzle, n e ≈ 1 – 5 × 10 19 cm -3 • Gas J et: • Q uadrupole magnets: permanent (PMQ s) & electromagnetic (EMQ s) • Beam profile monitors: pop-in Lanex screens / Ce:YAG crystals • Diagnostics: pop-in emittance mask & pop-in aluminium pellicle for transition radiation

  13. Electron Spectrometer • Designed by Allan Gillespie / Allan MacLeod • Built by Sigmaphi (France) Dual function device High resolution chamber Resolution – design ~ 0.1% Electron energy up to 105 MeV (B max = 1.65 T) High energy chamber Uses upstream quadrupoles to aid focusing Energy resolution ~0.2 – 10% (energy dependent) Electron energy up to ~ 660 MeV (B max = 1.65 T) Ce:YAG crystal 300 × 10 × 1 mm 14-bit PGR Grasshopper camera not shown

  14. Experimental Results – beam pointing 5 mrad • 500 consecutive shots • narrow divergence (~2 mrad) beam • wide divergence halo • θ X = (7 ± 3) mrad, θ Y = (3 ± 2) mrad • 8 mrad acceptance angle for EMQ s • 25% pointing reduction with PMQ s installed no PMQs PMQs in

  15. Experimental Results – PMQs • 1.5 T magnets (similar to the MPQ design) • Triplet settings for collimation of the “main peak” monoenergetic electron bunch • Swirls due to low energy halo electrons no PMQs PMQs in

  16. Experimental Results – energy stability Electron Spectrometer: 200 consecutive shots (spectrum on 196 shots) 69 90 124 185 Energy (MeV)

  17. 69 Energy (MeV) 90 124 185 100 consecutive shots Mean E 0 = (137 ± 4) MeV 2.8% stability

  18. Experimental Results – charge LANEX 2 Imaging Plate All screens now calibrated

  19. QUADS QUADS NO Experimental Results – energy spectra I QUADS QUADS NO

  20. Simulations of electron spectrometer response • General Particle Tracer (GPT) code • Analytical B field (fringe field responsible for the butterfly profile at 0% spread) electron beam energy = 83 MeV r.m.s. source size = 2 μ m spectrometer field = 0.59 T emittance ε N = 0.5 π mm mrad zero energy spread NO QUADS electron beam energy = 83 MeV QUADS r.m.s. source size = 2 μ m spectrometer field = 0.59 T zero energy spread i.e. to measure small spreads, emittance must be small!

  21. Experimental Results – energy spectra I I • Scaling of central energy and energy spread with charge Beam loading Beam loading • W iggins et al., PPCF 52 , 124032 (2010).

  22. Experimental Results – energy spectra I I I σ γ / γ MEAS σ γ / γ MEAS = 0.7% = 0.4% simulation simulation at 85 MeV at 146 MeV

  23. Experimental Results – energy spectra I I I E 0 = 172 MeV meas. σ E = 1.3 MeV meas. σ γ / γ = 0.75% E 0 = 210 MeV accelerating gradient ≈ 1 GeV/cm • 2mm gas jet: • A hint of a fixed absolute energy spread ~ 0.6-0.8 MeV

  24. Experimental Results – transverse emittance • Pepper pot mask technique σ x θ x <x> ∝ I*x - averaged σ x x ′ <x’> ∝ I*( θ x + σ x ) – averaged x Emittance (rms): ε x, rms = [<x 2 > <x’ 2 > - <xx’> 2 ] 1/2 Direct Calculation: x (Zhang FERMILAB-TM-1988) • First generation mask with hole φ ~ 55 μ m (b) x' [mrad] 3 2 • divergence 4 mrad 1 • hole size correction 0 -1.0 -0.5 0.0 0.5 1.0 • limited by detection system x [mm] -1 • ε N < (5.5 ± 1) π mm mrad -2 -3 0 50000 100000 counts

  25. Experimental Results – transverse emittance • Second generation mask with hole φ ~ 25 μ m and improved detection system • divergence 2-4 mrad for this run with 125 MeV electrons • average ε N = (2.0 ± 0.6) π mm mrad • best ε N = (1.0 ± 0.1) π mm mrad ε N , X > ε N , Y • Elliptical beam: False colour image of an electron beam with and • Resolution limited without the pepper‐pot mask.

  26. Experimental Results – transverse emittance • Measured emittance consistent with ~ 1 fs bunch • θ ∝ Q 1/2 scaling: implies constant σ z • θ ∝ Q 1/3 scaling: very slow increase of σ z with Q • Brunetti et al., Phys. Rev. Lett. 105 , 215007 (2010). • Experiments with third generation mask in progress.

  27. State of play • Measured low σ γ / γ < 1 % ( → 0% with spectrometer response) • Measured ε N = 1 π mm mrad (detector-limited, inferred ~0.5 π mm mrad) • Measured σ τ = 2 fs • Measured charge Q = 1-5 pC • W hy do we get these high quality beams? • O perating in a near-threshold, low charge regime. • Use PIC simulations and reduced models to understand our accelerator. • Injection of electrons from a small volume of phase-space. • Reduced model in progress.

  28. Phase-space distribution Measured beam profile PI C simulations of our LWFA

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